R is both a strongly functional programming language and a general environment for statistical exploration of data sets. As an environment, R allows you to create many graphical representations of data from a custom command line. See Part 1 of this series -- as well as Cameron Laird's article on R (both listed in Resources) -- for more on R and its background, as well as information on the platforms R runs on and the many packages available for it.
As with the interactive shells of Python, Ruby, wish for Tcl/Tk, or
many Lisp environments, the R shell is a great way to explore
operations -- command recall and editing let you try variations on
commands. In contrast to many other programming language interactive
shells, but in keeping with the data-centric nature of R, the R shell
will optionally save a complete environment (one per working
directory). A command history is a useful part of this: it can be
examined or modified in the file .Rhistory. But the major aspect of
saving an environment is the working data that is saved, in binary
form, to .RData. Incidentally, judicious use of the rm() command
can stop the saved data environment from growing unboundedly
(remove() is a synonym for rm()).
This article is a second installment on R. The first part introduced some basics of R's datatypes -- starting with vectors, but also including multidimensional arrays (2-D arrays are known as "matrices"), data frames for "smart" tables, lists for heterogeneous collections, and so on. The prior installment also performed some basic statistical analysis and graphing on a large data set that coauthor Brad had on hand: a one-year history of temperatures around Brad's house, taken at three-minute intervals. Like a lot of data sets in the real world, we either know of or suspect flaws and anomalies in Brad's temperature data -- in fact, part of this second installment will try to make sense of suspicious qualities of the data.
In general, the current article will do two things. First, we will continue to use the data set introduced in the first installment to explore the R language itself in more detail than we did last time. Second, we will examine general patterns in the data and show how to find them using R.
The (GPL'd) R programming language has two parents: S/S-PLUS and Scheme
(Lisp). The connection with Scheme is particularly worth emphasizing here,
as
the functional programming aspects of R come from the Scheme side of the
family.
Careful readers
might have noticed something oddly missing from the first
installment's examples: flow control! That lacuna will be continued
into this article as well. In point of fact, R has perfectly good
if, else, while, and for commands, all of them pretty much
just like the same-spelled command in Python. (Other languages spell
the same commands a bit differently.) Throw in repeat, break,
next, and switch
for a moderate amount of redundancy.
Programmers of imperative languages will be surprised by what you can
do without flow control; they'll be even more surprised at how much
easier many tasks are without it!
True to its functional programming heritage, you can do most everything you want to do in R using plain declarative statements. Two features of R make imperative flow control superfluous in most cases. In the first place, you have already seen that most operations on collection objects work elementwise. There is no need to manually loop through a vector of data to do something to its elements, as you can simply do something to all the elements of a vector:
Listing 1. Elementwise operations in R
> a = 1:10 # Range of numbers 1 through 10 > b = a+5 # Add 5 to each element > b # Show b vector [1] 6 7 8 9 10 11 12 13 14 15 |
Or you can operate selectively only on elements with certain indices, by using an "index array":
Listing 2. Using index arrays to select elements
> c = b # Make a (lazy) copy of b > pos = c(1,2,3,5,7) # Change the prime indices > c[pos] = c[pos]*10 # Reassign to indexed positions > c # Show c vector [1] 60 70 80 9 100 11 120 13 14 15 |
Or, maybe best of all, you can use a syntax much akin to list comprehensions in Haskell or Python, and only operate on elements that have a desired property:
Listing 3. Using predicates to select elements
> d = c > d[d %% 2 == 0] = -1 # Reassign -1 to all even elements > d [1] -1 -1 -1 9 -1 11 -1 13 -1 15 |
Very astute readers may have noticed that these examples use =, whereas
most of those in the last installment used <-. The equal sign does the same
thing as the assignment arrow, but may only be used at the top-level
scope, not also in nested expressions. If in doubt, the arrow is
safer.
In the first installment, we read approximately the first 170
thousand
readings at
each of four locations into a data frame using the function
read.table(). However, for more convenient access to the individual
temperature series, we copied the columns of data into vectors named
for the location they measure: outside,
livingroom,
basement, and
lab.
Remember
also that some of the data points were missing in each sequence:
sometimes the recording computer was down; sometimes instruments
failed; not all four thermometers came online on exactly the same day;
and so on. In other words, our temperature data is a lot like
real-life data you are likely to work with.
In our initial exploration of the temperature data sets, we noticed an anomaly while plotting histograms. There appears to be a large spike in outside temperature right near 24 degrees Celsius. Our first guess was that this spike represented occasional transpositions of the temperature readings, where one of the inside temperatures would be recorded in the outside log (and the outside, correspondingly, in one of the inside logs). As a way of exploring R, let us see if we can prove or disprove this explanation.
A first step in exploring anomalous data is just finding it. Specifically, a single point anomaly will be marked by a sudden fluctuation in temperature on each side of a data point. And even more specifically, we will expect both neighbors of an anomalous point to be either strongly higher or strongly lower than the candidate point. For example, the simple sequence of temperatures (at three minute intervals) "20, 16, 13" represent an unusually fast drop in temperature, but do not suggest a single point error at the middle reading. Of course, we do not a priori preclude the existence of other types of errors or oddities that pertain to more than just isolated readings.
Our first thoughts for identifying odd readings turned to the complex. Maybe we could look for high frequency components in Fourier transforms on the sequences. Or maybe we could perform analytic derivatives on the temperature vectors (probably second derivative to get the inflection). Or still yet, we might try convolutions on the temperature vectors. All of these options are built in to R. But after letting such lofty thoughts bounce around in our heads, we decided to settle down to earth. The simple pattern we are looking for is temperature readings that have large scalar differences from their neighbors. In other words, we can use the magic of subtraction.
The trick we will use to find all the differences among neighboring data points is to create a data frame whose columns in a given row correspond to the prior, current, and following data point. This lets us filter the data frame as a whole, selecting rows of possible interest.
Listing 4. Finding single-point oddities in outside temperatures
> len <- length(outside) # Shorthand name for scalar length of vector > i <- 1:(len-2) # Shorthand vector of data frame rows nums > # Create a data frame for window of measurements per row > odf <- data.frame(lst=outside[1:(len-2)], + now=outside[2:(len-1)], + nxt=outside[3:len] ) > # Create vector of local temperature fluctuations, add to data frame > odf$flux <- (odf[i,"now"]*2) - (odf[i,"lst"] + odf[i,"nxt"]) > odf2 <- odf[!is.na(odf$flux),] # Exclude "Not Available" readings > oddities <- odf2[abs(odf2$flux) > 6,] # It's odd if flux is over 6 |
So, what do we have after our filter? Let us take a look:
Listing 5. Eyeballing "oddities" in outside temperatures
> oddities
lst now nxt flux
2866 21.3 15.0 14.9 -6.2
79501 -1.5 -6.2 -4.1 -6.8
117050 21.2 24.6 21.6 6.4
117059 20.6 23.4 20.1 6.1
127669 24.1 21.2 24.7 -6.4
127670 21.2 24.7 21.5 6.7
|
It turns out we have several readings with a high fluctuation from their neighbors. But most of them do not look like very likely candidates for transposed readings. For example, at time step 79501, the temperature 6.2 is surrounded by two distinctly warmer temperatures. But it seems quite unlikely that any of these was an indoor temperature -- a particularly chilly breeze is a more plausible explanation.
It still looks quite conceivable that we had transpositions around time step 117059 or 12670. The middle temperatures are right near that indoor 24, and the neighboring readings, while definitely non-freezing, are distinctly lower. Maybe we have some springtime transpositions.
Wrapping useful operations in a function
What we would like to know now is whether our small number of
candidate transpositions show up in the other readings. If we find a
"missing" outdoor temperature in one of the indoor sites, it strongly
supports our hypothesis. But we do not really want to retype the
complete set of steps just replacing outside with lab everywhere.
What we really should have done is parameterize the whole sequence of
steps in a reusable function:
Listing 6. Parameterizing flux detector as a function
oddities <- function(temps, flux) {
len <- length(temps)
i <- 1:(len-2)
df <- data.frame(lst=temps[1:(len-2)],
now=temps[2:(len-1)],
nxt=temps[3:len])
df$flux <- (df[i,"now"]*2) - (df[i,"lst"] + df[i,"nxt"])
df2 <- df[!is.na(df$flux),]
oddities <- df2[abs(df2$flux) > flux,]
return(oddities)
}
|
Once we have a function, it is much easier to filter on different data
sets and fluctuation thresholds. It turns out that running
oddities(lab,6) does not produce any time steps that match the
candidate transpositions on the outside (neither does the same thing
with livingroom or basement). But a look at lab temperatures
produces something of its own surprise:
Listing 7. Huge temperature variations in the lab
> oddities(lab, 30)
lst now nxt flux
47063 19.9 -2.6 19.5 -44.6
47268 17.7 -2.6 18.2 -41.1
84847 17.1 -0.1 17.0 -34.3
86282 14.9 -1.0 14.8 -31.7
93307 14.2 -6.4 14.1 -41.1
|
These sorts of changes are not what we would expect. Maybe the best explanation is that Brad sometimes opened the lab window in the dead of winter. If so, coauthor David marvels at the efficiency of Brad's furnace in restoring full heat within three minutes of airing out a room.
Maybe looking the underlying full data for a curious time step will clear things up:
Listing 8. Full temperature set near step 47063
> glarp[47062:47066,]
timestamp basement lab livingroom outside
47062 2003-10-31T17:07 21.5 20.3 21.8 -2.8
47063 2003-10-31T17:10 21.3 19.9 21.2 -2.7
47064 2003-10-31T17:13 20.9 -2.6 20.9 -2.6
47065 2003-10-31T17:16 20.8 19.5 20.8 -2.6
47066 2003-10-31T17:19 20.5 19.4 20.7 -2.8
|
First thing, we notice that the time steps returned by the oddities()
function have an off-by-one error. Oh yeah, we used an offset to get
a window for each data frame row. But the full data itself tends to
promote the "opening a door" idea -- Halloween eve at 5 in the evening
can be pretty cold in Colorado, in fact it might be right when
trick-or-treaters show up at Brad's door (and receive candy for three
minutes). So maybe this mystery is solved.
Still, what about the mystery that started our exploration? Why is there such a spike around 24 degrees in outdoor temperatures? Maybe we should look at the histogram with some more care. In particular, we can use predicative criteria to index a vector, and narrow our histogram to just the temperature range of interest:
Listing 9. Narrowing the temperature histogram
hist(outside[outside < 26 & outside > 23],
breaks=90, col="green" border="blue")
|
Figure 1. Outside histogram for narrow temperature range
Looking at a close-up of the temperature spike, we see distinct troughs right next to the spike. It looks like if you would smooth the few tenths-of-a-degree region right around 24.7 degrees, you would almost get the expected occurrences. Which brings us back, most likely, to odd rounding behavior within the thermometer instrument. Well, probably -- we are still not sure. And even with some smoothing, there would still be a slight spike.
Intermediate statistical analysis
One of R's strengths is its ability to calculate linear, as well as
nonlinear regression models. To see a simple example, let us create
two vectors. x will be sample times in days measured from the
beginning of the data set, and y will be the corresponding outside
temperatures.
Listing 10. Creating regression vectors
> y <- glarp$outside > x <- 1:length(y)/(24*60/3) |
We can fit a line to this data with:
Listing 11. Fitting a linear regression to series
> l1 = lm(y ~ x)
> summary(l1)
Call:
lm(formula = y ~ x)
Residuals:
Min 1Q Median 3Q Max
-29.4402 -7.4330 0.2871 7.4971 23.1355
Coefficients:
Estimate Std. Error t value Pr(>|t|)
(Intercept) 10.2511014 0.0447748 228.95 <2e-16 ***
x -0.0037324 0.0002172 -17.19 <2e-16 ***
---
Signif. codes: 0 `***' 0.001 `**' 0.01 `*' 0.05 `.' 0.1 ` ' 1
Residual standard error: 9.236 on 169489 degrees of freedom
Multiple R-Squared: 0.00174, Adjusted R-squared: 0.001734
F-statistic: 295.4 on 1 and 169489 DF, p-value: < 2.2e-16
|
The "~" syntax denotes a formula object. This in effect asks R to find
the coefficients A and B that minimize sum((y[i]-(A*x[i]+B))^2).
The best fit is when A is -0.0037324 (very close to flat slope), and B
is 10.2511014. Note that the residual standard error is 9.236, which is
about the same size as the standard deviation in y to begin with. This
tells us that a simple linear function of time is an extremely bad
model for outside temperature.
A better model might be to use sine and cosine functions with a periods of 1 day and 1 year. This we can do by changing the formula to:
Listing 12. Attempting trigonometric curve fitting
> l2 = lm(y ~ +I(sin(2*pi*x/365)) +I(cos(2*pi*x/365)) + +I(sin(2*pi*x)) +I(cos(2*pi*x)) ) |
This formula syntax is a little tricky: inside the I() calls, the
arithmetic symbols have their usual meanings, so the first I(), for
example, means: 2 times pi times x, divided by 365. The "+" signs
in front of the I() calls indicate not addition, but that the factor
following the + should be included in the model. The result can, as
usual, be displayed with the summary() command
Listing 13. Trigonometric regression results
> summary(l2)
Call:
lm(formula = y ~ +I(sin(2 * pi * x/365)) +I(cos(2 * pi * x/365))
+I(sin(2 * pi * x)) +I(cos(2 * pi * x)))
Residuals:
Min 1Q Median 3Q Max
-21.7522 -3.4440 0.1651 3.7004 17.0517
Coefficients:
Estimate Std. Error t value Pr(>|t|)
(Intercept) 9.76817 0.01306 747.66 <2e-16 ***
I(sin(2 * pi * x/365)) -1.17171 0.01827 -64.13 <2e-16 ***
I(cos(2 * pi * x/365)) 10.04347 0.01869 537.46 <2e-16 ***
I(sin(2 * pi * x)) -0.58321 0.01846 -31.59 <2e-16 ***
I(cos(2 * pi * x)) 3.64653 0.01848 197.30 <2e-16 ***
---
Signif. codes: 0 `***' 0.001 `**' 0.01 `*' 0.05 `.' 0.1 ` ' 1
Residual standard error: 5.377 on 169486 degrees of freedom
Multiple R-Squared: 0.6617, Adjusted R-squared: 0.6617
F-statistic: 8.286e+04 on 4 and 169486 DF, p-value: < 2.2e-16
|
The residual error is still large (5.377), but we console ourselves in the fact that Colorado weather is notoriously unpredictable.
R provides still more tools for time series analysis. For example, we can plot the autocorrelation function for the living room temperature:
Listing 14. Autocorrelation on livingroom temperature
> acf(ts(glarp$livingroom, frequency=(24*60/3)), + na.action=na.pass, lag.max=9*(24*60/3)) |
Figure 2. Autocorrelation graph for livingroom
The embedded ts() function creates a time series object out of the
vector glarp$livingroom. The sampling frequency is specified in
samples per day. Not surprisingly, the temperature is strongly
correlated when the shift is an integer number of days. Note also the
slightly larger peak at seven days. This is caused by the fact that Brad's
thermostat sets the temperature differently on weekends (when Brad is
usually out of the house during the day), resulting in
slightly larger correlation with a seven-day window.
So far, we have used R for analyses of patterns and anomalies in a data set that has precisely the sort of gaps and potential problems that affect almost all real-world scientific data. This installment also explored how R's functional programming style aids in rapid exploration of patterns and data and analytic scenarios. Part 3 of this series will continue down the path of finding patterns in large data sets, using ever more sophisticated statistical techniques (but still only barely touching on the wealth of facilities in R as a whole).
- The first installment (developerWorks, September 2004) in this series introduced R and touched lightly on some of its features and language characteristics.
- Cameron Laird's Server clinic: R handy for crunching data (developerWorks, July 2003) gives a good overview of R (as well as S) and has a wealth of resources.
- Visit the home page for the R
Project for Statistical Computing. This R Web site contains extensive documentation, everything from tutorials to complete API descriptions. Two documents of
particular interest to those readers first encountering R are:
- An Introduction to R (PDF format)
- R Data Import/Export (PDF format)
- Several readers of David's Charming Python column, being
Python users,
have expressed a particular fondness for the Python binding to R.
Actually, there are two of them: RPy, and the older RSPython, which is also good (but David's impression is that the RPy binding is better). Either one of these bindings lets you call the full range of R functions transparently from Python code, using Python objects as
arguments to the functions.
-
For what it is worth, on most systems you can launch a browser with
generated HTML pages for R documentation by entering
help.start()at the R command line. -
A summary of the history of S and S-Plus is available online.
-
David wrote a Charming Python installment on
Numerical
Python, which has a similar feel and many of the same capabilities as
R (R is considerably more extensive, though).
-
The temperature data and the Python script for converting the initial
log format to a nicer tabular format are available for download:
- Find more resources for Linux™ developers in the developerWorks Linux zone.
- Download no-charge trial versions of IBM middleware products that run on Linux, including WebSphere® Studio Application Developer, WebSphere Application
Server, DB2® Universal Database, Tivoli® Access Manager, and Tivoli Directory Server,
and explore how-to articles and tech support, in the Speed-start your Linux app section of developerWorks.
- Get involved in the developerWorks community by participating in
developerWorks blogs.
- Browse for books on these and other technical topics.

To David Mertz, all the world is a stage; and his career is devoted to providing marginal staging instructions. Suggestions and recommendations on his articles are welcome. You can reach David at mertz@gnosis.cx; you can investigate all aspects of his life at his personal Web page. Check out his book, Text Processing in Python.
Brad has been doing UNIX® systems administration and network engineering for about 14 years at what used to be three different companies. He is currently working on a Ph.D. in Applied Mathematics at the University of Colorado in Boulder, and pays the bills by doing UNIX support for the Computer Science department.



